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Ames Research Center Image Library
by NASA/Ames Research Center
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CVSRF (crew Vehicle Systems Research Facility) N=257 High-Bay, T-NASA simulation HUD (heads up displays)
NASA Images
by NASA/NCSA University of Illinois
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This animation flies through the cosmic web of the early universe. At the end, we see the Hubble Space Telescope collecting data points.Launched in 1990, the Hubble Space Telescope (HST) has revolutionized astronomy by providing unprecedented views of the Universe. Hubble's spectral range extends from the ultraviolet, through the visible, and into the near-infrared. NASA will fly a servicing mission in 2008 to bring two new science instruments to Hubble - the Cosmic Origins Spectrograph and the...
Topics: HDTV, Hubble Space Telescope, HST, Astrophysics, SM4, Early Universe, Cosmology, Universe, What --...
Source: http://svs.gsfc.nasa.gov/goto?10118
NASA Images
by NASA/JPL-Caltech
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Close-up views of gullies, craters and ice layers, courtesy of NASA's Mars Reconnaissance Orbiter. Master: DVCPro HD. Audio 1: Mono mix. 2: Mono mix.
Topic: What -- Mars
NASA Images
by NASA/Glenn Research Center
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eye 22
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Open Source Foil Journal Bearing
NASA Images
by NASA/Glenn Research Center
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Enhanced Zero Gravity Locomotion (eZLS)
NASA Images
by NASA
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KENNEDY SPACE CENTER, FLA. -- Casting a brilliant reflection in the water near Launch Pad 39A at NASA's Kennedy Space Center, space shuttle Discovery trails a column of fire as it roars toward space on mission STS-120 to the International Space Station. Liftoff of Discovery was on time at 11:38:19 a.m. EDT. The mission is the 23rd assembly flight to the space station and the 34th flight for Discovery. The STS-120 payload is the Italian-built U.S. Node 2, called Harmony. During the 14-day...
Topics: What -- Space Shuttle Orbiter, What -- Discovery, What -- STS-120, What -- International Space...
Source: http://mediaarchive.ksc.nasa.gov/detail.cfm?mediaid=34020
NASA Images
by NASA
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KENNEDY SPACE CENTER, FLA. -- Space Shuttle Discovery has arrived at Launch Pad 39A. Discovery arrived at its seaside launch pad around noon and was hard down at 1:15 p.m. First motion out of the Vehicle Assembly Building was at 6:47 a.m. EDT. Rollout is a milestone for Discovery's launch to the International Space Station on mission STS-120, targeted for Oct. 23. The crew will be delivering and installing the Italian-built U.S. Node 2, named Harmony. The pressurized module will act as an...
Topics: What -- Space Shuttle Orbiter, What -- Discovery, What -- International Space Station (ISS), What...
Source: http://mediaarchive.ksc.nasa.gov/detail.cfm?mediaid=33625
NASA Images
by NASA
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KENNEDY SPACE CENTER, FLA. -- A dolphin surfaces in the Launch Complex 39 Area turn basin at NASA's Kennedy Space Center. The turn basin was carved out of the Banana River when Kennedy Space Center was built. Dolphins frequent bays and coastlines, usually in depths under 20 meters. While some pods take up permanent residence and establish home waters, others are migratory and swim considerable distances from coast to coast. Dolphins are a frequent sight in the rivers around Kennedy, which...
Topic: Where -- Kennedy Space Center (KSC)
Source: http://mediaarchive.ksc.nasa.gov/detail.cfm?mediaid=34144
NASA Images
by NASA
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KENNEDY SPACE CENTER, FLA. -- A dolphin's dorsal fin cuts through the water in the Launch Complex 39 Area turn basin at NASA's Kennedy Space Center. The turn basin was carved out of the Banana River when Kennedy Space Center was built. Dolphins frequent bays and coastlines, usually in depths under 20 meters. While some pods take up permanent residence and establish home waters, others are migratory and swim considerable distances from coast to coast. Dolphins are a frequent sight in the rivers...
Topic: Where -- Kennedy Space Center (KSC)
Source: http://mediaarchive.ksc.nasa.gov/detail.cfm?mediaid=34145
NASA Images
by *Video Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and G. Bacon (STScI [ http://www.stsci.edu/ ]) Selected still images from this video: (click to enlarge): [ http://hubblesite.org/newscenter/archive/releases/2007/16/video/a/still/1/ ] [ http://hubblesite.org/newscenter/archive/releases/2007/16/video/a/still/2/ ] [ http://hubblesite.org/newscenter/archive/releases/2007/16/video/a/still/3/ ]
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*Description*:> In celebration of the 17th anniversary of the launch and deployment of NASA's Hubble Space Telescope, a team of astronomers is releasing one of the largest panoramic images ever taken with Hubble's Advanced Camera for Surveys. It is a 50-light-year- wide view of the central region of the Carina Nebula where a maelstrom of star birth is taking place. This is a color version of a zoom into and pan across the heart of the Carina Nebula. The nebula's fantasy-like landscape is...
Topics: What -- Hubble Space Telescope (HST), What -- Advanced Camera for Surveys, What -- Camera 2, What...
Source: http://hubblesite.org/newscenter/archive/releases/2007/16/video/a/
NASA Images
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Technical facts about this news release: About the Object Object Description: Planetary Nebulae Object: He 2-47 What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. The colorful, intricate shapes in these NASA Hubble Space Telescope images reveal how the glowing gas ejected by dying Sun-like stars evolves dramatically over time. These gaseous clouds, called planetary nebulae, are created when stars in the last stages of life cast off their...
Topics: What -- Hubble Space Telescope (HST), What -- Sun, What -- Wide Field Planetary Camera 2, What --...
Source: http://hubblesite.org/newscenter/archive/releases/2007/33/image/b/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and the Hubble Heritage [ http://heritage.stsci.edu/ ] (STScI [ http://www.stsci.edu/ ]/AURA [ http://www.aura-astronomy.org/ ])-ESA [ http://www.spacetelescope.org/ ]/Hubble Collaboration *Acknowledgment:* R. Chandar (University of Toledo) and J. Miller (University of Michigan)
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*Description*: Resembling festive lights on a holiday wreath, this NASA/ESA Hubble Space Telescope image of the nearby spiral galaxy M74 is an iconic reminder of the impending season. Bright knots of glowing gas light up the spiral arms, indicating a rich environment of star formation. Messier 74, also called NGC 628, is a stunning example of a "grand-design" spiral galaxy that is viewed by Earth observers nearly face-on. Its perfectly symmetrical spiral arms emanate from the central...
Topics: M74, NGC 628, What -- Hubble Space Telescope (HST), What -- Earth, What -- Constellation, What --...
Source: http://hubblesite.org/newscenter/archive/releases/2007/41/image/a/
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio
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This movie shows the Sun from the two STEREO spacecraft using the 171 Å filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe<sup>+8</sup>=Fe IX, Fe<sup>+9</sup>=Fe X) which forms at temperatures above 1.3x10<sup>6</sup>K, and flows along the magnetic field lines of the solar active regions. New regions of solar activity come into view as the Sun rotates left to right. Note: This...
Topics: HDTV, Magnetic Fields, Solar Rotation, Sun, Earth Science, Sun-earth Interactions, Solar Activity,...
Source: http://svs.gsfc.nasa.gov/goto?3421
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio
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Solar Dynamics Observatory (SDO) will dramatically increase our ability to collect data about the Sun. This visualization compares the temporal and spatial resolution of SOHO/EIT with TRACE. SDO will enable TRACE-like image and temporal resolution over the entire solar disk. This movie opens with a full-disk view of the Sun in ultraviolet light (195 Ôæå__ngstroms) from SOHO/EIT using the traditional TRACE 'gold' color table. We zoom in on the active region on the western limb where the TRACE...
Topics: HDTV, Solar Active Region, Solar Ultraviolet, Sun, Earth Science, Sun-earth Interactions, Solar...
Source: http://svs.gsfc.nasa.gov/goto?3435
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio
movies
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NASA's TRMM spacecraft observed this view of Hurricane Dean on August 19, 2007. At this time the storm was classified as a dangerous category four with sustained winds of 125 knots (138 mph). The cloud cover is taken by TRMM's Visible and Infrared Scanner(VIRS) and the GOES spacecraft. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar(PR) instruments. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. Blue...
Topics: Atmospheric science, HDTV, Natural hazards, What -- Tropical Rainfall Measuring Mission (TRMM),...
Source: http://svs.gsfc.nasa.gov/goto?3447
NASA Images
movies
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Left side view of Stereo Shots of Mars Phoenix beginning of Gantry Roll. Rollback occurred at 10:27 pm EDT at Cape Canaveral Florida at Pad 17A of a Delta Heavy. Master: DVCPro LP. Audio 1: Mono mix 2: Mono mix.
Topics: What -- STEREO, What -- Mars, What -- Phoenix, Where -- Florida
NASA Images
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Technical facts about this news release: About the Object Object Name: MC2 1635+119, MC2 1635+11.9 Object Description: Shell structure around a QSO Position (J2000): R.A. 16h 37m 46s.51 Dec. +11° 49' 49".34 Constellation: Hercules Dimensions: This image is roughly 1.2 arcminutes (600,000 light-years or 180 kiloparsecs) wide. Redshift The object has a redshift, z = 0.146. About the Data Data Description: The Hubble image was created from HST data from proposal 10421: G. Canalizo...
Topics: What -- Constellation, What -- Hercules, What -- Hubble Space Telescope (HST), Where -- California,...
Source: http://hubblesite.org/newscenter/archive/releases/2007/39/image/b/
NASA Images
by NASA/JPL-Caltech/Z. Balog (Univ. of Ariz./Univ. of Szeged)
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This infrared image from NASA's Spitzer Space Telescope shows the Rosette nebula, a pretty star-forming region more than 5,000 light-years away in the constellation Monoceros. In optical light, the nebula looks like a rosebud, or the "rosette" adornments that date back to antiquity. But lurking inside this delicate cosmic rosebud are so-called planetary "danger zones" (see sphere illustrations). These zones surround super hot stars, called O-stars (blue stars inside...
Topics: What -- Infrared Array Camera (IRAC), What -- Spitzer Space Telescope, What -- Constellation, What...
Source: http://sscws1.ipac.caltech.edu/Imagegallery/image.php?image_name=ssc2007-08b
Ames Research Center Image Library
by NASA/Ames Research Center
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From left: Data Parallel Line Relaxation (DPLR) software team members Kerry Trumble, Deepak Bose and David Hash analyze and predict the extreme environments NASAÔø_Ôø_Ôø_s space shuttle experiences during its super high-speed reentry into EarthÔø_Ôø_Ôø_s atmosphere.
Topic: What -- Space Shuttle Orbiter
NASA Images
by NASA
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Technical facts about this news release: About the Object Object Name: Saturn Object Description: Planet Distance: The semi-major axis of Saturn's orbit about the sun is 9.5 Astronomical Units (A.U.) or roughly 1.4 billion km. Dimensions: The planet (without rings) has a diameter of roughly 75,000 miles (120,000 km) at the equator. About the Data Data Description: The Hubble images and videos were created from HST data from proposal 6030: M. Tomasko and E. Karkoschka (University of Arizona);...
Topics: What -- Saturn, What -- Sun, What -- Hubble Space Telescope (HST), Where -- Arizona
Source: http://hubblesite.org/newscenter/archive/releases/2007/13/image/n/
NASA Images
by NASA/Solar & Heliospheric Observatory
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Solar study spacecraft from a number of missions observe the Sun in various wavelengths of light every day. This representative collage, made from images taken on November 25, 2007, suggests some (but not all) of the various missions and wavelengths that are captured and made available on the web daily. By observing in different wavelengths of light the instruments show different features of the Sun at different temperatures and elevations above the surface. And when you consider the two STEREO...
Topics: What -- Sun, What -- STEREO, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/30nov2007/
NASA Images
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Technical facts about this news release: About the Object Object Name: Extended Groth Strip, EGS Object Description: Optical Survey Position (J2000): R.A. 14h 17m Dec. +52° 30' Constellation: Ursa Major Dimensions: The Extended Groth Strip is 1.1 degrees long by 0.15 degrees wide (70.5 x 10.1 arcminutes, respectively). About the Data Data Description: The Hubble image was created from HST data from proposal 10134: M. Davis (University of California, Berkeley), M. Ashby (Harvard-Smithsonian...
Topics: What -- Constellation, What -- Ursa Major, What -- Hubble Space Telescope (HST), What -- Planck,...
Source: http://hubblesite.org/newscenter/archive/releases/2007/06/image/f/
NASA Images
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Technical facts about this news release: About this Survey Name: Cosmological Evolution Survey (COSMOS) Field Description: Astronomical Survey Position (J2000): R.A. 10h 00m 28s.6 Dec. +02° 12' 21".0 Constellation: Sextens Dimensions: The COSMOS survey field covers 2 square degrees. About the Data Mission: Hubble Subaru VLT XMM/Newton Survey Type: Optical Optical Spectral x-Ray Instrument: ACS/WFC Suprime-Cam VIMOS EPIC Principal Ivestigator: Scoville: 9822; 10092 Taniguchi Kneib Hasinger...
Topics: What -- Constellation, What -- Hubble Space Telescope (HST), What -- VLT, Where -- California
Source: http://hubblesite.org/newscenter/archive/releases/2007/01/image/h/
NASA Images
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Technical facts about this news release: About this Survey Name: Cosmological Evolution Survey (COSMOS) Field Description: Astronomical Survey Position (J2000): R.A. 10h 00m 28s.6 Dec. +02° 12' 21".0 Constellation: Sextens Dimensions: The COSMOS survey field covers 2 square degrees. About the Data Mission: Hubble Subaru VLT XMM/Newton Survey Type: Optical Optical Spectral x-Ray Instrument: ACS/WFC Suprime-Cam VIMOS EPIC Principal Ivestigator: Scoville: 9822; 10092 Taniguchi Kneib Hasinger...
Topics: What -- Constellation, What -- Hubble Space Telescope (HST), What -- VLT, Where -- California
Source: http://hubblesite.org/newscenter/archive/releases/2007/01/image/b/
NASA Images
by NASA
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Technical facts about this news release: About the Object Object Name: Saturn Object Description: Planet Distance: The semi-major axis of Saturn's orbit about the sun is 9.5 Astronomical Units (A.U.) or roughly 1.4 billion km. Dimensions: The planet (without rings) has a diameter of roughly 75,000 miles (120,000 km) at the equator. About the Data Data Description: The Hubble images and videos were created from HST data from proposal 6030: M. Tomasko and E. Karkoschka (University of Arizona);...
Topics: What -- Saturn, What -- Sun, What -- Hubble Space Telescope (HST), Where -- Arizona
Source: http://hubblesite.org/newscenter/archive/releases/2007/13/image/k/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and G. Bacon (STScI [ http://www.stsci.edu/ ]) Selected still images from this video: (click to enlarge): [ http://hubblesite.org/newscenter/archive/releases/2007/10/video/a/still/1/ ] [ http://hubblesite.org/newscenter/archive/releases/2007/10/video/a/still/2/ ] [ http://hubblesite.org/newscenter/archive/releases/2007/10/video/a/still/3/ ]
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*Description*:> A time-lapse sequence of 12 years of Hubble observing SN 1987A shows the onrushing stellar shock wave from the stellar explosion as it is slamming into, heating up, and illuminating the inner regions of the narrow ring surrounding the doomed star. Technical facts about this news release: About the Object Object Name: SN 1987A Object Description: Supernova in the Large Magellanic Cloud (LMC) Position (J2000): R.A. 05h 35m 28s.26 Dec. -69° 16' 13".0 Constellation: Dorado...
Topics: What -- Hubble Space Telescope (HST), What -- Constellation, What -- Dorado, Where -- Large...
Source: http://hubblesite.org/newscenter/archive/releases/2007/10/video/a/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and the Hubble Heritage [ http://heritage.stsci.edu/ ] Team (AURA [ http://www.aura-astronomy.org/ ]/STScI [ http://www.stsci.edu/ ])
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*Description*: NASA's Hubble Space Telescope took this true-color view of Jupiter in support of the New Horizons Mission. The image was taken with Hubble's Wide Field Planetary Camera 2 on February 17, 2007, using the planetary camera detector. Jupiter's trademark belts and zones of high- and low-pressure regions appear in crisp detail. Circular convection cells can be seen at high northern and southern latitudes. Atmospheric features as small as 250 miles (400 km) across can be discerned....
Topics: Jupiter, What -- Hubble Space Telescope (HST), What -- Jupiter, What -- New Horizons, What -- Wide...
Source: http://hubblesite.org/newscenter/archive/releases/2007/11/image/e/
NASA Images
by NASA
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Technical facts about this news release: About the Object Object Name: NGC 6397 Object Description: Globular Cluster Position (J2000): R.A. 17h 40m 41s.36 Dec. -53° 40' 25".3 Constellation: Ara Distance: 8,500 light-years (2.6 kiloparsecs) About the Data Data Description: This image was created from HST data from proposal 10424: H. Richer (University of British Columbia), P. Guhathakurta (University of California, Santa Cruz), R.M. Rich (University of California, Los Angeles), J. Anderson...
Topics: What -- Constellation, What -- Ara, What -- Hubble Space Telescope (HST), What -- Columbia, Where...
Source: http://hubblesite.org/newscenter/archive/releases/2007/42/image/c/
NASA Images
by *Photo Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and N. Pirzkal (STScI [ http://www.stsci.edu/ ]/ESA [ http://www.spacetelescope.org/ ])
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*Description*: Building block galaxy at redshift of 4.88 from Hubble Ultra Deep Field image. Technical facts about this news release: About the Object Object Description: Galaxies in the Hubble Ultra Deep Field (HUDF) Position (J2000): R.A. 03h 32m 40s.0 Dec. -27° 48' 00" Constellation: Fornax Dimensions: The full HUDF image is 3 arcminutes square. About the Data Data Description: The science data were selected based on findings from The Grism-ACS Program for Extragalactic Science...
Topics: What -- Constellation, What -- Fornax, What -- Hubble Space Telescope (HST), What -- NICMOS, What...
Source: http://hubblesite.org/newscenter/archive/releases/2007/31/image/d/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and G. Bacon (STScI [ http://www.stsci.edu/ ])
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Technical facts about this news release: About the Object Object Name: Carina Nebula, NGC 3372 Object Description: Emission Nebula in the Milky Way Galaxy Position (J2000): R.A. 10h 44m Dec. -59° 53' Constellation: Carina Distance: Approximately 7,500 light-years (2,300 parsecs) Dimensions: This image is roughy 25 arcminutes (53 light-years or 16 parsecs) wide. About the Data Data Description: This color image combines many exposures from Hubble Space Telescope's Advanced Camera for Surveys...
Topics: What -- Carina, What -- Constellation, What -- Wide Field Planetary Camera 2, What -- Hubble Space...
Source: http://hubblesite.org/newscenter/archive/releases/2007/16/image/s/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], Digitized Sky Survey Consortium, and the STScI [ http://www.stsci.edu/ ]-Google Partnership
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*Description*: Screen capture of the Orion constellation border and numerous astronomical objects located in the direction of that constellation. Technical facts about this news release: Back to entire collection [ http://hubblesite.org/newscenter/archive/releases/index/23/ ] Next release [ http://hubblesite.org/newscenter/archive/releases/2007/30/ ] Previous release [ http://hubblesite.org/newscenter/archive/releases/2007/32/ ] *News Release Number:*: STScI-2007-22c
Topics: What -- Orion, What -- Constellation, What -- Earth
Source: http://hubblesite.org/newscenter/archive/releases/2007/22/image/c/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], S. Beckwith (STScI [ http://www.stsci.edu/ ]) and the HUDF Team
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*Description*: This tapestry of galaxies represents a small piece of the Hubble Ultra Deep Field (HUDF), taken from September 2003 through January 2004 by the Hubble Space Telescope. The HUDF is the deepest visible-light view of the cosmos and includes galaxies of various ages, sizes, shapes, and colors. The image is part of an exploration activity for students at a NASA education workshop planned for Queen Elizabeth II's visit. Students will study the HUDF image and classify the galaxies by...
Topics: Hubble Ultra Deep Field, HUDF, What -- Hubble Space Telescope (HST), What -- Visible Light, What --...
Source: http://hubblesite.org/newscenter/archive/releases/2007/21/image/a/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], A. Zezas and J. Huchra (Harvard-Smithsonian Center for Astrophysics)
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*Description*: Hubble's high-resolution images of distinct regions contained within M81 illustrate various structures contained within the spiral galaxy. [Left] The inner bulge and nucleus of M81 are relatively structure free, except for fine dust lanes that wind into the center. Several whitish-colored concentrations of stars, known as globular clusters are easily visible. [Middle] A string of star-forming regions show along a spiral arm, their glowing hydrogen gas appears green in color. A...
Topics: M81, NGC 3031, Bode's Galaxy, What -- Constellation, What -- Ursa Major, What -- Hubble Space...
Source: http://hubblesite.org/newscenter/archive/releases/2007/19/image/b/
NASA Images
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Technical facts about this news release: About the Object Object Name: Jupiter Object Description: Planet Distance: The semi-major axis of Jupiter's orbit about the sun is 5.2 Astronomical Units (778 million km or 483 million miles). Dimensions: The planet has a diameter of roughly 88,789 miles (142,984 km) at the equator. About the Data/Images Proposal: 11096: K. Noll (STScI), H. Weaver (Johns Hopkins University/Applied Physics Laboratory), A. Simon-Miller (NASA Goddard Space Flight Center),...
Topics: What -- Jupiter, What -- Sun, Where -- Goddard Space Flight Center (GSFC), Where -- Hamilton, Where...
Source: http://hubblesite.org/newscenter/archive/releases/2007/25/image/b/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], A. Zezas and J. Huchra (Harvard-Smithsonian Center for Astrophysics)
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*Description*: Southern extremity of the galaxy M81. Technical facts about this news release: About the Object Object Name: M81, NGC 3031, Bode's Galaxy Object Description: Spiral Galaxy Position (J2000): R.A. 09h 55m 33s Dec. +69° 03' 55" Constellation: Ursa Major Distance: Approximately 11.6 million light-years (3.6 megaparsecs) Dimensions: This image is roughy 19 arcminutes (64,000 light-years or roughly 20 kiloparsecs) wide. About the Data Data Description: The ACS data was from the...
Topics: M81, NGC 3031, Bode's Galaxy, What -- Constellation, What -- Ursa Major, What -- Hubble Space...
Source: http://hubblesite.org/newscenter/archive/releases/2007/19/image/h/
NASA Images
by NASA/Solar & Heliospheric Observatory
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On May 9, 2007 two smaller coronal mass ejections (CMEs)burst out from the Sun. The first one headed to the left; the second, to the right, suggesting that they perhaps did not share the same source. Since CMEs of any visible size have been fairly rare over the past several months, the fact that we see two in one day is noteworthy. These were observed with our LASCO C2 coronagraph, one of two coronagraphs on SOHO. These are our best tools for observing solar storms in the corona. We continue to...
Topics: What -- Sun, What -- SOHO, What -- Earth
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/11may2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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Grab your 3D glasses (if you have any around) and get ready for something never seen before by anyone. We proudly present to you the first ever actual 3D stills and movies of the Sun from the twin STEREO spacecraft. These images were just released on April 23, 2007. And even if you can't see them in 3D, you can still enjoy the unsurpassed levels of detail in these 2D, full disk solar images with twice the resolution of SOHO. The still image taken on March 24, 2007 shows a coronal hole (darker...
Topics: What -- Sun, What -- STEREO, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/23apr2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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This is one of the clearest and most engaging clips of solar plasma shimmying and arcing above the edge of the Sun that we have ever been able to view (May 9-10, 2007). With STEREO's high frame rate (an image every few minutes) and high resolution, we can zoom in on areas of interest yet maintain image clarity. This large sunspot was just rotating to the edge of the Sun when we zoomed in on its action for about 18 hours. The active region, a hot bed of intense magnetic forces, is the source of...
Topics: What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/18may2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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Just as 2006 was about to end, the Sun decided to blast out two more CMEs, perhaps as a symbol of New Year's revelry. At any rate, in the span of 24 hours (Dec. 30-31, 2006), two separate CMEs blew out to the right of the Sun at close to identical locations. The first event was a good-sized solar storm with a classical, expanding bulbous shape. The second, smaller event was more linear and directional as it left the Sun. Incidentally, Mercury can once again (remember its transit in November?)...
Topics: What -- Sun, What -- Mercury, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/05jan2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 15
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Over a period of four days (July 27 - 31, 2007) two active regions can be seen by SOHO communicating with each other magnetically. While the areas remained fairly stable, in that they did not generate any solar storms, the magnetic field lines of connection between them shift and sway most of the time. Like two magnets that sit near each other, the magnetic fields of the active regions share a dynamic interplay that is fun to watch. While we cannot actually see magnetic field lines, we can see...
Topics: What -- SOHO, What -- Sun
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/15aug2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
image
eye 18
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A close-up of an active region of the Sun from STEREO's Ahead spacecraft in extreme ultraviolet revealed an interesting, yet subtle, phenomenon. Besides a pair of small eruptions over this 40-hour period (Aug. 23-24, 2007), one small point was the source of a steady outpouring of material in all directions around it during the whole time, almost like a sparkler. It may not be an actual outflow into the solar wind - these are likely just the footprints of longer loops that continue upwards at...
Topics: What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/31aug2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 20
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The Earth passed through a stream of solar wind that flowed out of this expansive coronal hole (seen in lower central area of the Sun in still on January 14, 2006). Coronal holes appear as a dark area of the Sun when viewed in ultraviolet light (as it is here) and in X-rays. Since coronal holes are 'open' magnetically, strong solar wind gusts can escape from them and carry solar particles out to our magnetosphere and beyond. Solar wind streams take several days to travel from the Sun to Earth,...
Topics: What -- Earth, What -- Sun, What -- SOHO, Where -- Wisconsin
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/19jan2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 14
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A well-positioned and substantial coronal hole can be seen (right of center) in this (November14, 2007) image by SOHO. Coronal holes appear as the dark areas when viewed in this wavelength (284 Angstrom) of extreme ultraviolet light and others as well. It has been rotating around towards the center of the Sun over the past week or so. Since coronal holes are 'open' magnetically, strong solar wind gusts can escape from them and carry solar particles out to our magnetosphere and beyond. Solar...
Topics: What -- SOHO, What -- Sun, What -- Earth
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/16nov2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
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Over a five-day stretch (Nov. 30 - Dec. 4, 2007) SOHO observed two remarkably similar coronal mass ejections (CMEs). The first one blew out to the right from the Sun as a familiar arch- shaped, bulbous CME. Just four days later another, slightly larger, CME headed out to the right in just about the same direction and similarly shaped. With the Sun being near its minimum period of activity, it was a little surprising to see two CMEs in this short a span of time. With the brilliant Sun blocked...
Topics: What -- SOHO, What -- Sun
Source: http://sohowww.nascom.nasa.gov/pickoftheweek/old/07dec2007/
NASA Images
by NASA/Solar & Heliospheric Observatory
movies
eye 71
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Erupting prominences (Mar. 30 - Apr. 6, 1998)
Source: http://sohowww.nascom.nasa.gov/gallery/Movies/filaments.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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SOHO on the Atlas II-AS (AC-121), Cape Canaveral Air Station, 2 December 1995. SOHO was launched on 2 December 1995, 03:08 EST (08:08 UT).
Topics: What -- SOHO, What -- Atlas
Source: http://sohowww.nascom.nasa.gov/gallery/Spacecraft/PL95C-11589.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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SOHO on the Atlas II-AS (AC-121), Cape Canaveral Air Station, 2 December 1995. SOHO was launched on 2 December 1995, 03:08 EST (08:08 UT).
Topics: What -- SOHO, What -- Atlas
Source: http://sohowww.nascom.nasa.gov/gallery/Spacecraft/PL95C-11587.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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Active region loops observed on the West limb.
Topic: What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/cds010.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 12
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A LASCO C2 "running difference" image showing a "halo" CME blast beginning its journey towards Earth. With the LASCO C2 instrument providing a perspective of about six solar, the Sun is seen hurtling particles into space during a CME on 7 April 1997. The image compares one image to the preceding one and highlights the areas of change between the two. This gives a clearer representation of the dynamics of this "halo event," so called because the circular area of the...
Topics: What -- Earth, What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/images/c2dblast.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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Observing the Sun with a spectrometer like CDS one can derive the intensity and velocity distribution of the O V 629 ? line formed at approximately 230 000 K in AR8737. Pixels with Doppler shifts corresponding to a velocity greater than ?40 km/s is fully red/blue. Contours outline areas with velocities exceeding ?50 km/s. The velocities are calculated relative to the part of the solar disk (to the left) that is within the field of view.
Topics: What -- Sun, What -- Spectrometer, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/cds028.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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Ratio of EIT full Sun images in Fe XII 195A to Fe IX/X 171A as recorded on 12 May 1996 between 06:53 and 06:59 UT. This line ratio gives an indication of the temperature distribution in the Sun's corona with dark areas being cooler regions and bright areas being hotter.
Topics: What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/eit010.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 19
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Large, eruptive prominence in He II at 304Ôø_, with an image of the Earth added for size comparison. This prominence from 24 July 1999 is particularly large and looping, extending over 35 Earths out from the Sun. Erupting prominences (when Earthward directed) can affect communications, navigation systems, even power grids, while also producing auroras visible in the night skies.
Topics: What -- Earth, What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/images/eit99promclose.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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Cutaway - The three major zones of the Sun's internal structure are shown in this cutaway of an EIT 304 image. The core (temperature of 15 million degrees) is where the nuclear fusion occurs. In the large radiative zone the plasma and energy are gradually moved outwards from the core over a period of thousands of years. Finally, the hot plasma is cycled through a convection process (represented by the series of circles) in the convection zone up to the surface and out into space.
Topic: What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/images/cutaway00.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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ERNE/HED measurements of a ring-like anisotropy of 16-20 MeV protons accelerated by an IP-shock on 11 August 2000. The instrument's angular resolution enables it to see far more accurate directional intensity distributions than any other particle instrument in this energy scale. To the area outside the HED viewcone (marked with a semi-circular boundary) an estimate of the distribution is drawn, based on the high resolution pitch-angle distribution measured by the instrument.
Topic: What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/Particle/ern010.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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SOHO-EIT image in resonance lines of eight and nine times ionized iron (Fe IX/X) at 171 Angstroms in the extreme ultraviolet showing the solar corona at a temperature of about 1 million K. This image was recorded on 11 September 1997. It is dominated by two large active region systems, composed of numerous magnetic loops.
Topic: What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/eit028.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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Large sunspot group -- Active region 9169 was the host of the largest sunspot group observed so far during the current solar cy Joseph B. Gurman Normal Joseph B. Gurman 1 2001-02-02T20:26:00Z 2001-02-02T20:32:00Z 1 75 428 NASA GSGC 3 1 525 9.2511 800x600 0 0 Large sunspot group -- Active region 9169 was the host of the largest sunspot group observed so far during the current solar cycle. On 23 September 2000, the sunspot area within the group spanned 2,140 millionths of the visible solar...
Topic: What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/images/sunspot00.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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These combined images display UV light emitted by the the solar corona on 17 August 1996. The solar disk image is from the EIT instrument aboard SOHO, and the extended solar corona (outside the black ring about 0.5 solar radii from the disk) is from the UVCS instrument aboard SOHO. The color in the latter image represents the total UV intensity emitted by highly ionized oxygen atoms (O VI, or O 5+) in the corona. The blue-white rays are lines of magnetic force from a theoretical model of the...
Topics: What -- SOHO, What -- Sun, What -- Polar
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/uvcs07.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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The figure is a composite image taken by three SOHO instruments at the time of the 21 April 2002 solar flare. The green image of the solar disk at the time of the flare was taken by EIT in light emitted by iron ions at about 2 million degrees Kelvin. The blue/white image of a coronal mass ejection associated with the flare was taken by LASCO in visible light. UVCS images of the region outlined in white were made in light from four ultraviolet emissions, each showing threads of ejected material...
Topics: What -- SOHO, What -- Visible Light
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/uvc009.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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MDI Sunspot size winner -- Active region 10486 became the largest sunspot seen by SOHO, It unleashed a spectacular show on 28 October 2003. An X 17.2 flare, the second largest flare observed by SOHO and the third largest ever recorded, blasted off a strong high energy proton event and a fast-moving Coronal Mass Ejection. The spot occupied an area equal to about 15 Earths, a size not seen since 1989. It later fired off the largest X-ray flare recorded, on 4 November 2003.
Topics: What -- SOHO, What -- FAST
Source: http://sohowww.nascom.nasa.gov/gallery/images/mdi20031028.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 24
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The LASCO C2 frame was selected to show Comet SOHO-6, one of numerous sungrazing comets discovered by LASCO, as its head enters the equatorial solar wind region. It eventually plunged into the Sun. This image of the solar corona on 23 December 1996 also shows the inner streamer belt along the Sun's equator, where the low latitude solar wind originates and is accelerated. Over the polar regions, one sees the polar plumes all the way out to the edge of the field of view. The field of view of this...
Topics: What -- SOHO, What -- COMETS, What -- Sun, What -- Polar
Source: http://sohowww.nascom.nasa.gov/gallery/images/xmascomet.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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SWAN Lyman-alpha whole sky map in ecliptic coordinates. Two areas were not covered for safety reasons, around the Sun (at left) and around the anti-solar direction (at right). The color is coding the intensity, in counts per second per pixel (one square degree), which corresponds to 1.3 Rayleigh. A number of UV hot stars can be identified, tracing the galactic plane. The rest of the ubiquitous emission is due to solar UV Lyman alpha photons, backscattered by Hydrogen atoms in the solar system....
Topics: What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/Particle/swa001.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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eye 22
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MDI Single Dopplergram Minus 45 Image Average Subtracting an average solar velocity image observed over 45 minutes from a single velocity image reveals the surface motions associated with sound waves traveling through the Sun's interior. The smallscale light and dark regions represent the up and down motions of the hot gas near the Sun's surface. The pattern falls off towards the limb because the acoustic waves are primarily radial.
Topic: What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/Helioseismology/mdi002.html
NASA Images
by NASA/Solar & Heliospheric Observatory
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The Sun observed by SUMER on 2-4 March 1996 in the emission line of He I at 584.3 A, formed in the upper chromosphere at about 20,000 K. The picture was put together from eight horizontal raster scans in alternating directions, starting in the solar NE. Each raster scan includes 1600 exposures, lasting 7 seconds each. The picture is shown in bins of 4x4 pixels, one pixel being approx. 1 arcsec. The brightest pixels correspond to an intensity of more than 70 counts/line/arcsec (with a maximum of...
Topics: What -- Sun, What -- SOHO
Source: http://sohowww.nascom.nasa.gov/gallery/SolarCorona/sum005.html
NASA Images
by NASA/Stennis Space Center
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Pratt & Whitney Rocketdyne's Jeff Hansell, right, explains functions of a space shuttle main engine to Pearl River Community College Aviation Maintenance Technology Program students. Christopher Bryon, left, of Bay St. Louis, Ret Tolar of Kiln, Dan Holston of Baxterville and Billy Zugg of Long Beach took a recent tour of the SSME Processing Facility and the E-1 Test Complex at Stennis Space Center in South Mississippi. The students attend class adjacent to the Stennis International Airport...
Topics: Pearl River Community College, Aviation Maintenance students, E Test Complex, space shuttle main...
Source: http://www.ssc.nasa.gov/sirs/
NASA Images
by NASA/Stennis Space Center
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Michael Sandras, a member of the Pontchartrain Astronomical Society, explains his solar telescope to students of Second Street in Bay St. Louis, Hancock County and Nicholson elementary schools in StenniSphere's Millennium Hall on April 10. The students participated in several hands-on activities at Stennis Space Center's Sun-Earth Day celebration.
Topics: Pontchartrain Astronomical Society, Stennis Space Center's Sun-Earth Day, StenniSphere's Millennium...
Source: http://www.ssc.nasa.gov/sirs/
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio Historic calving front locations courtesy of Anker Weidick and Ole Bennike
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Jakobshavn Isbrae is located on the west coast of Greenland at Latitude 69 N. The ice front, where the glacier calves into the sea, receded more than 40 km between 1850 and 2006. Between 1850 and 1964 the ice front retreated at a steady rate of about 0.3 km/yr, after which it occupied approximately the same location until 2001, when the ice front began to recede again, but far more rapidly at about 3 km/yr. After 2004, the glacier began retreating up its two main tributaries: one to the north,...
Topics: Cryology, Earth Science, Cryosphere, Earth Science, Cryosphere, Snow/Ice, Earth Science,...
Source: http://svs.gsfc.nasa.gov/goto?3395
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio
movies
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This movie shows the Sun from the two STEREO spacecraft using the 284 Ôæå__ngstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe<sup>+14</sup>=Fe XV), which forms at temperatures above 2x10<sup>6</sup>K, and flows along the magnetic field lines of the solar active regions. New regions come into view as the Sun rotates. Note: Left-eye movie of the Sun in ultraviolet. Animator: Eric DeJong (NASA/JPL...
Topics: HDTV, Magnetic Fields, Solar Rotation, Sun, Earth Science, Sun-earth Interactions, Solar Activity,...
Source: http://svs.gsfc.nasa.gov/goto?3424
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio
movies
eye 90
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This movie shows the Sun from the two STEREO spacecraft using the 284 Ångstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe<sup>+14</sup>=Fe XV), which forms at temperatures above 2x10<sup>6</sup>K, and flows along the magnetic field lines of the solar active regions. New active regions come into view as the Sun rotates. Note: Left-eye movie of the Sun at 284 Ångstroms, ultraviolet light....
Topics: HDTV, Magnetic Fields, Solar Rotation, Sun, Earth Science, Sun-earth Interactions, Solar Activity,...
Source: http://svs.gsfc.nasa.gov/goto?3425
NASA Images
by NASA/Goddard Space Flight Center Scientific Visualization Studio
movies
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Sea ice is frozen seawater floating on the surface of the ocean. Some sea ice is semi-permanent, persisting from year to year, and some is seasonal, melting and refreezing from season to season. The sea ice cover reaches its minimum extent at the end of each summer and the remaining ice is called the perennial ice cover. This animation shows a 3-year moving average of the perennial ice cover, or minimum sea ice concentration, for from 1979-1981 through 2004-2006. The area of the perennial ice...
Topics: Cryology, HDTV, Earth Science, Cryosphere, Earth Science, Cryosphere, Sea Ice, Earth Science,...
Source: http://svs.gsfc.nasa.gov/goto?3445
NASA Images
movies
eye 497
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A series of severe Martian summer dust storms has affected Mars rover Opportunity. The dust in the Martian atmosphere over Opportunity has blocked 99 percent of the direct sunlight, leaving only the limited diffuse sky light to power the rover. Master: DVCPro HD. Audio 1: Mono mix. 2: Mono mix.
Topics: What -- Mars, What -- Opportunity
NASA Images
image
eye 23
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Technical facts about this news release: About the Object Object Name: HD 15115 Object Description: Star with Debris Disk Position (J2000): R.A. 02h 26m 16s.28 Dec. +06° 17' 32".9 Constellation: Cetus Distance: 150 light-years (45 parsecs) Dimensions: This image is 23 arcseconds (roughly 1000 Astronomical Units) across. About the Data Data Description: This image was created from data from the HST proposal 10896: P. Kalas, J. Graham, M. Fitzgerald (University of California, Berkeley)....
Topics: What -- Constellation, What -- Cetus, What -- Hubble Space Telescope (HST), Where -- California
Source: http://hubblesite.org/newscenter/archive/releases/2007/28/image/c/
NASA Images
by *Credit:* NASA [ http://www.nasa.gov/ ], ESA [ http://www.spacetelescope.org/ ], and M. Brown (California Institute of Technology)
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*Description*: [Left] - This is an image of the dwarf planet Eris (center) and its satellite Dysnomia (at 9 o'clock position) taken with NASA's Hubble Space Telescope on Aug. 30, 2006. Hubble observations were obtained on Dec. 3, 2005 and Aug. 30, 2006 using the Advanced Camera for Surveys. The Hubble images were combined with images from the Keck telescopes taken on Aug. 20, 21, 30, and 31 to measure the satellite's orbit and calculate a mass for Eris, which is the largest dwarf planet in the...
Topics: 2003 UB313, Eris, What -- Eris, What -- Hubble Space Telescope (HST), What -- Advanced Camera for...
Source: http://hubblesite.org/newscenter/archive/releases/2007/24/image/a/
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 13
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Three tests performed of skid gear at 8.1-, 10.0- and 12.7-ft/s. Tests conducted in building 1297c.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Three tests performed of skid gear at 8.1-, 10.0- and 12.7-ft/s. Tests conducted in building 1297c.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 12
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Three tests performed of skid gear at 8.1-, 10.0- and 12.7-ft/s. Tests conducted in building 1297c.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 11
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Three tests performed of skid gear at 8.1-, 10.0- and 12.7-ft/s. Tests conducted in building 1297c.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 16
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Photographed in building 1244 Annex and NTF bulding 1236.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 32
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Portrait of Wayne R. Mantay
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 44
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Titanium Biaxial
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 56
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Titanium Biaxial
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 11
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Portrait of Patricia L. Donnington
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 16
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IRVIN Aerospace Airbag Testing
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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IRVIN Aerospace Airbag Testing
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 16
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 13
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 13
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 13
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 12
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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In briefing at Building 1219, room 225. Tours of building 1232A, 8 Foot HTT bldg 1265, Simulator Cockpit Motion Facility bldg 1268D, NTF bldg 1236, cafeteria working lunches, session throughout center.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 11
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In briefing at Building 1219, room 225. Tours of building 1232A, 8 Foot HTT bldg 1265, Simulator Cockpit Motion Facility bldg 1268D, NTF bldg 1236, cafeteria working lunches, session throughout center.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 11
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In briefing at Building 1219, room 225. Tours of building 1232A, 8 Foot HTT bldg 1265, Simulator Cockpit Motion Facility bldg 1268D, NTF bldg 1236, cafeteria working lunches, session throughout center.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 12
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In briefing at Building 1219, room 225. Tours of building 1232A, 8 Foot HTT bldg 1265, Simulator Cockpit Motion Facility bldg 1268D, NTF bldg 1236, cafeteria working lunches, session throughout center.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 14
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.
Langley Research Center Media Archive
by NASA/Langley Research Center
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eye 16
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Returned specimens from MISSE 3 & 4. Photographed 09/07/07 through 10/07/07 in building 1250 - Clean Room.